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Bienvenue sur la collection HAL de la Maison de la Simulation, laboratoire commun au CEA, au CNRS, à l'Université Paris-Saclay et à l'Université Versailles Saint-Quentin. Elle est spécialisée dans le calcul haute performance et les simulations numériques en lien étroit avec les applications physiques, le génie logiciel parallèle, les modèles de programmation, les techniques de visualisation, l'intelligence artificielle et l'informatique quantique.
Dépôts récents
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Sara Moukir, Miwako Tsuji, Nahid Emad, Mitsuhisa Sato, Stephane Baudelocq. Advancements in traffic simulations with multiMATSim’s distributed framework. ICAART 2024 - the 16th International Conference on Agents and Artificial Intelligence, Feb 2024, rome, Italy. pp.374-385, ⟨10.5220/0012452600003636⟩. ⟨hal-04496277⟩
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Sara Moukir, Nahid Emad, Stéphane Baudelocq. A high performance algorithmic variant of MATSim road traffic simulator. IPDPSW 2023 - IEEE International Parallel and Distributed Processing Symposium Workshops, May 2023, St petersburg, United States. pp.914-922, ⟨10.1109/IPDPSW59300.2023.00149⟩. ⟨hal-04496008⟩
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Thomas Padioleau, Pascal Tremblin, Edouard Audit, Pierre Kestener, Samuel Kokh. A High-performance and Portable All-Mach Regime Flow Solver Code with Well-balanced Gravity. Application to Compressible Convection. The Astrophysical Journal, 2019, 875 (2), pp.128. ⟨10.3847/1538-4357/ab0f2c⟩. ⟨cea-04381512⟩
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Sohvi Luukkonen, Luc Belloni, Daniel Borgis, Maximilien Levesque. Predicting hydration free energies of the freesolv database of drug-like molecules with molecular density functional theory. Journal of Chemical Information and Modeling, 2020, 60 (7), pp.3558-3565. ⟨10.1021/acs.jcim.0c00526⟩. ⟨cea-02909000⟩
Pour toute question : hal@cea.fr
Nombre de documents
275
Nombre de notices
117
Indicateur d'Open Access
85 %
Evolution des dépôts
mots clés
Godunov-type scheme
Domain decomposition
Insider threat
Asynchronous communication
Methods statistical
Gravitational effects
Planets and satellites atmospheres
Dynamic processes
Conservation laws
Calcul haute performance
Well-balanced property
Infrared planetary systems
High angular resolution
FFT
Planets and satellites formation
Unite and conquer
Ensemble learning
ISM kinematics and dynamics
Unite and Conquer
Two-phase flows
Low Froude
Astrometry
GPU computing
Big data
Astrophysics - Astrophysics of Galaxies
Gas dynamics
Accretion disks
Compressible two-phase flow
Interferometers-planets and satellites
Astrochemistry
Planets and satellites fundamental parameters
Iterative methods
Instrumentation
Cybersecurity
Planets and satellites gaseous planets
Water
Exascale
ISM individual objects Orion B
Stars massive
Brown dwarfs
Shallow water equations
Techniques spectroscopic
Methods data analysis
Detection-techniques
Dask
HII regions
Supercapacitors
AMITEXFFTP
Methods numerical
Solvation
Complex and heterogeneous dynamic system
ISM structure
Accretion
Energy
Geometric multigrid
High performance computing
Hydrodynamics
Laser
65Y05
Convection
Boosting
Planets and satellites interiors
OpenMP
Schrödinger equation
Level-Set
Plasma physics
MPI
Astrophysics - Solar and Stellar Astrophysics
Big data analysis
Hyperbolic systems
Magnetohydrodynamics
Low Mach correction
Supernovae general
Linear algebra
Radiative transfer
Sparse matrix
Approximate Riemann solver
High Performance Computing
Adaptive optics-instrumentation
Planets and satellites composition
Astrophysics - Earth and Planetary Astrophysics
Epidemic
Aerodynamics
Sharp interface
ISM molecules
Stars formation
Parallel computing
HPC
Low-Mach correction
Bagging
Surface tension
Efficiency
CUDA
ISM clouds
Linear systems
Large time steps
Data parallelism
Turbulence
Ghost Fluid method
Electron